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Precipitate formation in austenitic stainless steel welds

Journal Article · · Scr. Metall.; (United States)
Recent research efforts have revealed many of the factors which control the hotcracking susceptibility of austenitic stainless steel weld metals. It is generally agreed that the segregation of impurity elements to solidification grain boundaries is a primary cause of the hot-cracking tendency of these alloys in that elements such as phosphorus and sulfur form low melting point eutectics with the metal matrix. Furthermore, these elements can also degrade cracking resistance by lowering the surface tension of the interdendritic fluids to which they segregate. In the case of phosphide precipitation in austenitic stainless steel weld metal, there is apparently some question in the literature as to the specific phosphide formed. This study was undertaken to determine the microstructural relationships, relative to phosphide formation, pertaining to hot-cracking of austenitic stainless steel weld metals. The results confirm that phosphides of the type (Fe, Cr)/sub 3/P form in austenitic stainless steel welds. These phosphides appear at both eutecticferrite/austenite interfaces and along solidification hot-cracks, where they most likely form via an eutectic reaction. These results are inconsistent with those of Brooks et al. in that no evidence of either the MP or MP/sub 3/ phosphide was found. No reference could be found, either in the published literature or in standard compilations of crystallographic information, to verify the existence of a CrP/sub 3/ phase, suggesting that the theory of chromium depletion (CrP/sub 3/ vs. CrS) needs further substantiation before it is accepted.
Research Organization:
Sandia National Laboratories, Albuquerque, NM
OSTI ID:
6325069
Journal Information:
Scr. Metall.; (United States), Journal Name: Scr. Metall.; (United States) Vol. 19:2; ISSN SCRMB
Country of Publication:
United States
Language:
English